LSSTApplications
18.0.0+106,18.0.0+50,19.0.0,19.0.0+1,19.0.0+10,19.0.0+11,19.0.0+13,19.0.0+17,19.0.0+2,19.0.0-1-g20d9b18+6,19.0.0-1-g425ff20,19.0.0-1-g5549ca4,19.0.0-1-g580fafe+6,19.0.0-1-g6fe20d0+1,19.0.0-1-g7011481+9,19.0.0-1-g8c57eb9+6,19.0.0-1-gb5175dc+11,19.0.0-1-gdc0e4a7+9,19.0.0-1-ge272bc4+6,19.0.0-1-ge3aa853,19.0.0-10-g448f008b,19.0.0-12-g6990b2c,19.0.0-2-g0d9f9cd+11,19.0.0-2-g3d9e4fb2+11,19.0.0-2-g5037de4,19.0.0-2-gb96a1c4+3,19.0.0-2-gd955cfd+15,19.0.0-3-g2d13df8,19.0.0-3-g6f3c7dc,19.0.0-4-g725f80e+11,19.0.0-4-ga671dab3b+1,19.0.0-4-gad373c5+3,19.0.0-5-ga2acb9c+2,19.0.0-5-gfe96e6c+2,w.2020.01
LSSTDataManagementBasePackage
|
Detect positive and negative sources on an exposure and return a new table.SourceCatalog. More...
Public Member Functions | |
def | __init__ (self, schema=None, kwds) |
Create the detection task. More... | |
def | run (self, table, exposure, doSmooth=True, sigma=None, clearMask=True, expId=None) |
def | display (self, exposure, results, convolvedImage=None) |
def | applyTempLocalBackground (self, exposure, middle, results) |
def | clearMask (self, mask) |
def | calculateKernelSize (self, sigma) |
def | getPsf (self, exposure, sigma=None) |
def | convolveImage (self, maskedImage, psf, doSmooth=True) |
def | applyThreshold (self, middle, bbox, factor=1.0) |
def | finalizeFootprints (self, mask, results, sigma, factor=1.0) |
def | reEstimateBackground (self, maskedImage, backgrounds) |
def | clearUnwantedResults (self, mask, results) |
def | detectFootprints (self, exposure, doSmooth=True, sigma=None, clearMask=True, expId=None) |
def | makeThreshold (self, image, thresholdParity, factor=1.0) |
def | updatePeaks (self, fpSet, image, threshold) |
def | tempWideBackgroundContext (self, exposure) |
Static Public Member Functions | |
def | setEdgeBits (maskedImage, goodBBox, edgeBitmask) |
Public Attributes | |
negativeFlagKey | |
Static Public Attributes | |
ConfigClass = SourceDetectionConfig | |
def | makeSourceCatalog = run |
An alias for run. More... | |
Detect positive and negative sources on an exposure and return a new table.SourceCatalog.
Detect positive and negative sources on an exposure and return a new table.SourceCatalog.
Create the detection task. Most arguments are simply passed onto pipe.base.Task.
schema | An lsst::afw::table::Schema used to create the output lsst.afw.table.SourceCatalog |
**kwds | Keyword arguments passed to lsst.pipe.base.task.Task.__init__. |
If schema is not None and configured for 'both' detections, a 'flags.negative' field will be added to label detections made with a negative threshold.
Run source detection and create a SourceCatalog of detections. Parameters ---------- table : `lsst.afw.table.SourceTable` Table object that will be used to create the SourceCatalog. exposure : `lsst.afw.image.Exposure` Exposure to process; DETECTED mask plane will be set in-place. doSmooth : `bool` If True, smooth the image before detection using a Gaussian of width ``sigma``, or the measured PSF width. Set to False when running on e.g. a pre-convolved image, or a mask plane. sigma : `float` Sigma of PSF (pixels); used for smoothing and to grow detections; if None then measure the sigma of the PSF of the exposure clearMask : `bool` Clear DETECTED{,_NEGATIVE} planes before running detection. expId : `int` Exposure identifier; unused by this implementation, but used for RNG seed by subclasses. Returns ------- result : `lsst.pipe.base.Struct` ``sources`` The detected sources (`lsst.afw.table.SourceCatalog`) ``fpSets`` The result resturned by `detectFootprints` (`lsst.pipe.base.Struct`). Raises ------ ValueError If flags.negative is needed, but isn't in table's schema. lsst.pipe.base.TaskError If sigma=None, doSmooth=True and the exposure has no PSF. Notes ----- If you want to avoid dealing with Sources and Tables, you can use detectFootprints() to just get the `lsst.afw.detection.FootprintSet`s.
The command line task interface supports a flag -d
to import debug.py from your PYTHONPATH
; see Using lsstDebug to control debugging output for more about debug.py files.
The available variables in SourceDetectionTask are:
display
This code is in measAlgTasks.py in the examples directory, and can be run as e.g.
Import the task (there are some other standard imports; read the file if you're confused)
We need to create our task before processing any data as the task constructor can add an extra column to the schema, but first we need an almost-empty Schema
We're now ready to process the data (we could loop over multiple exposures/catalogues using the same task objects). First create the output table:
And process the image
We can then unpack and use the results:
To investigate the Debug variables, put something like
into your debug.py file and run measAlgTasks.py with the –debug
flag.
Definition at line 168 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.__init__ | ( | self, | |
schema = None , |
|||
kwds | |||
) |
Create the detection task.
Most arguments are simply passed onto pipe.base.Task.
schema | An lsst::afw::table::Schema used to create the output lsst.afw.table.SourceCatalog |
**kwds | Keyword arguments passed to lsst.pipe.base.task.Task.__init__. |
If schema is not None and configured for 'both' detections, a 'flags.negative' field will be added to label detections made with a negative threshold.
Definition at line 265 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.applyTempLocalBackground | ( | self, | |
exposure, | |||
middle, | |||
results | |||
) |
Apply a temporary local background subtraction This temporary local background serves to suppress noise fluctuations in the wings of bright objects. Peaks in the footprints will be updated. Parameters ---------- exposure : `lsst.afw.image.Exposure` Exposure for which to fit local background. middle : `lsst.afw.image.MaskedImage` Convolved image on which detection will be performed (typically smaller than ``exposure`` because the half-kernel has been removed around the edges). results : `lsst.pipe.base.Struct` Results of the 'detectFootprints' method, containing positive and negative footprints (which contain the peak positions that we will plot). This is a `Struct` with ``positive`` and ``negative`` elements that are of type `lsst.afw.detection.FootprintSet`.
Definition at line 414 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.applyThreshold | ( | self, | |
middle, | |||
bbox, | |||
factor = 1.0 |
|||
) |
Apply thresholds to the convolved image Identifies ``Footprint``s, both positive and negative. The threshold can be modified by the provided multiplication ``factor``. Parameters ---------- middle : `lsst.afw.image.MaskedImage` Convolved image to threshold. bbox : `lsst.geom.Box2I` Bounding box of unconvolved image. factor : `float` Multiplier for the configured threshold. Return Struct contents ---------------------- positive : `lsst.afw.detection.FootprintSet` or `None` Positive detection footprints, if configured. negative : `lsst.afw.detection.FootprintSet` or `None` Negative detection footprints, if configured. factor : `float` Multiplier for the configured threshold.
Definition at line 570 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.calculateKernelSize | ( | self, | |
sigma | |||
) |
Calculate size of smoothing kernel Uses the ``nSigmaForKernel`` configuration parameter. Note that that is the full width of the kernel bounding box (so a value of 7 means 3.5 sigma on either side of center). The value will be rounded up to the nearest odd integer. Parameters ---------- sigma : `float` Gaussian sigma of smoothing kernel. Returns ------- size : `int` Size of the smoothing kernel.
Definition at line 462 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.clearMask | ( | self, | |
mask | |||
) |
Clear the DETECTED and DETECTED_NEGATIVE mask planes Removes any previous detection mask in preparation for a new detection pass. Parameters ---------- mask : `lsst.afw.image.Mask` Mask to be cleared.
Definition at line 449 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.clearUnwantedResults | ( | self, | |
mask, | |||
results | |||
) |
Clear unwanted results from the Struct of results If we specifically want only positive or only negative detections, drop the ones we don't want, and its associated mask plane. Parameters ---------- mask : `lsst.afw.image.Mask` Mask image. results : `lsst.pipe.base.Struct` Detection results, with ``positive`` and ``negative`` elements; modified.
Definition at line 705 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.convolveImage | ( | self, | |
maskedImage, | |||
psf, | |||
doSmooth = True |
|||
) |
Convolve the image with the PSF We convolve the image with a Gaussian approximation to the PSF, because this is separable and therefore fast. It's technically a correlation rather than a convolution, but since we use a symmetric Gaussian there's no difference. The convolution can be disabled with ``doSmooth=False``. If we do convolve, we mask the edges as ``EDGE`` and return the convolved image with the edges removed. This is because we can't convolve the edges because the kernel would extend off the image. Parameters ---------- maskedImage : `lsst.afw.image.MaskedImage` Image to convolve. psf : `lsst.afw.detection.Psf` PSF to convolve with (actually with a Gaussian approximation to it). doSmooth : `bool` Actually do the convolution? Set to False when running on e.g. a pre-convolved image, or a mask plane. Return Struct contents ---------------------- middle : `lsst.afw.image.MaskedImage` Convolved image, without the edges. sigma : `float` Gaussian sigma used for the convolution.
Definition at line 509 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.detectFootprints | ( | self, | |
exposure, | |||
doSmooth = True , |
|||
sigma = None , |
|||
clearMask = True , |
|||
expId = None |
|||
) |
Detect footprints on an exposure. Parameters ---------- exposure : `lsst.afw.image.Exposure` Exposure to process; DETECTED{,_NEGATIVE} mask plane will be set in-place. doSmooth : `bool`, optional If True, smooth the image before detection using a Gaussian of width ``sigma``, or the measured PSF width of ``exposure``. Set to False when running on e.g. a pre-convolved image, or a mask plane. sigma : `float`, optional Gaussian Sigma of PSF (pixels); used for smoothing and to grow detections; if `None` then measure the sigma of the PSF of the ``exposure``. clearMask : `bool`, optional Clear both DETECTED and DETECTED_NEGATIVE planes before running detection. expId : `dict`, optional Exposure identifier; unused by this implementation, but used for RNG seed by subclasses. Return Struct contents ---------------------- positive : `lsst.afw.detection.FootprintSet` Positive polarity footprints (may be `None`) negative : `lsst.afw.detection.FootprintSet` Negative polarity footprints (may be `None`) numPos : `int` Number of footprints in positive or 0 if detection polarity was negative. numNeg : `int` Number of footprints in negative or 0 if detection polarity was positive. background : `lsst.afw.math.BackgroundList` Re-estimated background. `None` if ``reEstimateBackground==False``. factor : `float` Multiplication factor applied to the configured detection threshold.
Definition at line 729 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.display | ( | self, | |
exposure, | |||
results, | |||
convolvedImage = None |
|||
) |
Display detections if so configured Displays the ``exposure`` in frame 0, overlays the detection peaks. Requires that ``lsstDebug`` has been set up correctly, so that ``lsstDebug.Info("lsst.meas.algorithms.detection")`` evaluates `True`. If the ``convolvedImage`` is non-`None` and ``lsstDebug.Info("lsst.meas.algorithms.detection") > 1``, the ``convolvedImage`` will be displayed in frame 1. Parameters ---------- exposure : `lsst.afw.image.Exposure` Exposure to display, on which will be plotted the detections. results : `lsst.pipe.base.Struct` Results of the 'detectFootprints' method, containing positive and negative footprints (which contain the peak positions that we will plot). This is a `Struct` with ``positive`` and ``negative`` elements that are of type `lsst.afw.detection.FootprintSet`. convolvedImage : `lsst.afw.image.Image`, optional Convolved image used for thresholding.
Definition at line 360 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.finalizeFootprints | ( | self, | |
mask, | |||
results, | |||
sigma, | |||
factor = 1.0 |
|||
) |
Finalize the detected footprints Grows the footprints, sets the ``DETECTED`` and ``DETECTED_NEGATIVE`` mask planes, and logs the results. ``numPos`` (number of positive footprints), ``numPosPeaks`` (number of positive peaks), ``numNeg`` (number of negative footprints), ``numNegPeaks`` (number of negative peaks) entries are added to the detection results. Parameters ---------- mask : `lsst.afw.image.Mask` Mask image on which to flag detected pixels. results : `lsst.pipe.base.Struct` Struct of detection results, including ``positive`` and ``negative`` entries; modified. sigma : `float` Gaussian sigma of PSF. factor : `float` Multiplier for the configured threshold.
Definition at line 619 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.getPsf | ( | self, | |
exposure, | |||
sigma = None |
|||
) |
Retrieve the PSF for an exposure If ``sigma`` is provided, we make a ``GaussianPsf`` with that, otherwise use the one from the ``exposure``. Parameters ---------- exposure : `lsst.afw.image.Exposure` Exposure from which to retrieve the PSF. sigma : `float`, optional Gaussian sigma to use if provided. Returns ------- psf : `lsst.afw.detection.Psf` PSF to use for detection.
Definition at line 482 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.makeThreshold | ( | self, | |
image, | |||
thresholdParity, | |||
factor = 1.0 |
|||
) |
Make an afw.detection.Threshold object corresponding to the task's configuration and the statistics of the given image. Parameters ---------- image : `afw.image.MaskedImage` Image to measure noise statistics from if needed. thresholdParity: `str` One of "positive" or "negative", to set the kind of fluctuations the Threshold will detect. factor : `float` Factor by which to multiply the configured detection threshold. This is useful for tweaking the detection threshold slightly. Returns ------- threshold : `lsst.afw.detection.Threshold` Detection threshold.
Definition at line 797 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.reEstimateBackground | ( | self, | |
maskedImage, | |||
backgrounds | |||
) |
Estimate the background after detection Parameters ---------- maskedImage : `lsst.afw.image.MaskedImage` Image on which to estimate the background. backgrounds : `lsst.afw.math.BackgroundList` List of backgrounds; modified. Returns ------- bg : `lsst.afw.math.backgroundMI` Empirical background model.
Definition at line 681 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.run | ( | self, | |
table, | |||
exposure, | |||
doSmooth = True , |
|||
sigma = None , |
|||
clearMask = True , |
|||
expId = None |
|||
) |
Run source detection and create a SourceCatalog of detections. Parameters ---------- table : `lsst.afw.table.SourceTable` Table object that will be used to create the SourceCatalog. exposure : `lsst.afw.image.Exposure` Exposure to process; DETECTED mask plane will be set in-place. doSmooth : `bool` If True, smooth the image before detection using a Gaussian of width ``sigma``, or the measured PSF width. Set to False when running on e.g. a pre-convolved image, or a mask plane. sigma : `float` Sigma of PSF (pixels); used for smoothing and to grow detections; if None then measure the sigma of the PSF of the exposure clearMask : `bool` Clear DETECTED{,_NEGATIVE} planes before running detection. expId : `int` Exposure identifier; unused by this implementation, but used for RNG seed by subclasses. Returns ------- result : `lsst.pipe.base.Struct` ``sources`` The detected sources (`lsst.afw.table.SourceCatalog`) ``fpSets`` The result resturned by `detectFootprints` (`lsst.pipe.base.Struct`). Raises ------ ValueError If flags.negative is needed, but isn't in table's schema. lsst.pipe.base.TaskError If sigma=None, doSmooth=True and the exposure has no PSF. Notes ----- If you want to avoid dealing with Sources and Tables, you can use detectFootprints() to just get the `lsst.afw.detection.FootprintSet`s.
Definition at line 297 of file detection.py.
|
static |
Set the edgeBitmask bits for all of maskedImage outside goodBBox Parameters ---------- maskedImage : `lsst.afw.image.MaskedImage` Image on which to set edge bits in the mask. goodBBox : `lsst.geom.Box2I` Bounding box of good pixels, in ``LOCAL`` coordinates. edgeBitmask : `lsst.afw.image.MaskPixel` Bit mask to OR with the existing mask bits in the region outside ``goodBBox``.
Definition at line 875 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.tempWideBackgroundContext | ( | self, | |
exposure | |||
) |
Context manager for removing wide (large-scale) background Removing a wide (large-scale) background helps to suppress the detection of large footprints that may overwhelm the deblender. It does, however, set a limit on the maximum scale of objects. The background that we remove will be restored upon exit from the context manager. Parameters ---------- exposure : `lsst.afw.image.Exposure` Exposure on which to remove large-scale background. Returns ------- context : context manager Context manager that will ensure the temporary wide background is restored.
Definition at line 905 of file detection.py.
def lsst.meas.algorithms.detection.SourceDetectionTask.updatePeaks | ( | self, | |
fpSet, | |||
image, | |||
threshold | |||
) |
Update the Peaks in a FootprintSet by detecting new Footprints and Peaks in an image and using the new Peaks instead of the old ones. Parameters ---------- fpSet : `afw.detection.FootprintSet` Set of Footprints whose Peaks should be updated. image : `afw.image.MaskedImage` Image to detect new Footprints and Peak in. threshold : `afw.detection.Threshold` Threshold object for detection. Input Footprints with fewer Peaks than self.config.nPeaksMaxSimple are not modified, and if no new Peaks are detected in an input Footprint, the brightest original Peak in that Footprint is kept.
Definition at line 832 of file detection.py.
|
static |
Definition at line 262 of file detection.py.
|
static |
An alias for run.
Definition at line 358 of file detection.py.
lsst.meas.algorithms.detection.SourceDetectionTask.negativeFlagKey |
Definition at line 280 of file detection.py.